Jonathon Nosowitz
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View article: Investigating the Vertical Variability of Titan’s 14N/15N in HCN
Investigating the Vertical Variability of Titan’s 14N/15N in HCN Open
Titan’s substantial atmosphere is primarily composed of molecular nitrogen (N2) and methane (CH4), which are dissociated by solar UV photons and subsequently generate a vast chemical network of trace gases. The composition of Titan’s atmos…
View article: Temporal Variability of Titan’s Equatorial Zonal Winds Between 2012-2
Temporal Variability of Titan’s Equatorial Zonal Winds Between 2012-2 Open
Titan, Saturn’s largest satellite, is host to an intricate chemical and dynamical environment. Its atmosphere is composed primarily of molecular nitrogen (N2) and methane (CH4) that form the basis for a complex organic chemistry. But there…
View article: Improved Carbon and Nitrogen Isotopic Ratios for CH<sub>3</sub>CN in Titan’s Atmosphere Using ALMA
Improved Carbon and Nitrogen Isotopic Ratios for CH<sub>3</sub>CN in Titan’s Atmosphere Using ALMA Open
Titan, Saturn’s largest satellite, maintains an atmosphere composed primarily of nitrogen (N 2 ) and methane (CH 4 ) that leads to complex organic chemistry. Some of the nitriles (CN-bearing organics) on Titan are known to have substantial…
View article: Measuring Isotopic Ratios in Titan's Atmospheric Nitriles
Measuring Isotopic Ratios in Titan's Atmospheric Nitriles Open
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